Hogg 12 and NGC 3590: A new open cluster binary system candidate
We have obtained CCD UBVIKC photometry down to V ∼ 22.0 for the open clusters Hogg 12 and NGC 3590 and the fields surrounding them. Based on photometric and morphological criteria, as well as on the stellar density in the region, our evidence is sufficient to confirm that Hogg 12 is a genuine open c...
Guardado en:
| Autores principales: | Piatti, A.E., Claría, J.J., Ahumada, A.V. |
|---|---|
| Formato: | JOUR |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046280_v122_n891_p516_Piatti |
| Aporte de: |
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